Grain Evolution in B335? Models Meet Observations

Details Grain Evolution in B335? Models Meet Observations Grain Evolution in B335? Models Meet Observations

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aas...21116217t&link_type=abstract

American Astronomical Society, AAS Meeting #211, #162.17

Astronomy and Astrophysics

Astronomy

Scientific paper

B335, a nearly spherical, isolated, star-forming cloud is a natural target for studying the potential for grain evolution. Observations of the observed flux spectrum and surface brightness distribution in the infrared as well as H-K extinctions are compared to simulated observations produced via self-consistent radiative transfer models. Preliminary results suggest that grain evolution may be a key component to understanding the observed spectrum and surface brightness distribution.

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